<?xml version="1.0" encoding="UTF-8"?><!DOCTYPE article  PUBLIC "-//NLM//DTD Journal Publishing DTD v3.0 20080202//EN" "http://dtd.nlm.nih.gov/publishing/3.0/journalpublishing3.dtd"><article xmlns:mml="http://www.w3.org/1998/Math/MathML" xmlns:xlink="http://www.w3.org/1999/xlink" dtd-version="3.0" xml:lang="en" article-type="research article"><front><journal-meta><journal-id journal-id-type="publisher-id">AM</journal-id><journal-title-group><journal-title>Applied Mathematics</journal-title></journal-title-group><issn pub-type="epub">2152-7385</issn><publisher><publisher-name>Scientific Research Publishing</publisher-name></publisher></journal-meta><article-meta><article-id pub-id-type="doi">10.4236/am.2013.41010</article-id><article-id pub-id-type="publisher-id">AM-27131</article-id><article-categories><subj-group subj-group-type="heading"><subject>Articles</subject></subj-group><subj-group subj-group-type="Discipline-v2"><subject>Physics&amp;Mathematics</subject></subj-group></article-categories><title-group><article-title>
 
 
  MHD Free Convective Flow of Water near 4℃ past a Vertical Moving Plate with Constant Suction
 
</article-title></title-group><contrib-group><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>ichalis</surname><given-names>Xenos</given-names></name><xref ref-type="aff" rid="aff1"><sup>1</sup></xref><xref ref-type="corresp" rid="cor1"><sup>*</sup></xref></contrib><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Stelios</surname><given-names>Dimas</given-names></name><xref ref-type="aff" rid="aff2"><sup>2</sup></xref></contrib><contrib contrib-type="author" xlink:type="simple"><name name-style="western"><surname>Andreas</surname><given-names>Raptis</given-names></name><xref ref-type="aff" rid="aff1"><sup>1</sup></xref></contrib></contrib-group><aff id="aff1"><addr-line>Department of Mathematics, University of Ioannina, Ioannina, Greece</addr-line></aff><aff id="aff2"><addr-line>Instituto de Matemática, Estatística e Computa??o Científica, Universidade Estadual de Campinas,
Campinas, Brasil </addr-line></aff><author-notes><corresp id="cor1">* E-mail:<email>mxenos@cc.uoi.gr(IX)</email>;</corresp></author-notes><pub-date pub-type="epub"><day>25</day><month>01</month><year>2013</year></pub-date><volume>04</volume><issue>01</issue><fpage>52</fpage><lpage>57</lpage><history><date date-type="received"><day>November</day>	<month>9,</month>	<year>2012</year></date><date date-type="rev-recd"><day>December</day>	<month>9,</month>	<year>2012</year>	</date><date date-type="accepted"><day>December</day>	<month>16,</month>	<year>2012</year></date></history><permissions><copyright-statement>&#169; Copyright  2014 by authors and Scientific Research Publishing Inc. </copyright-statement><copyright-year>2014</copyright-year><license><license-p>This work is licensed under the Creative Commons Attribution International License (CC BY). http://creativecommons.org/licenses/by/4.0/</license-p></license></permissions><abstract><p>
 
 
  The aim of this work is the study of the magnetohydrodynamic (MHD) unsteady free convective flow of water near 4
  ℃
   past an infinitely vertical plate moving with constant velocity. The influence of constant uniform suction was also considered. The partial differential equations (PDEs) and their initial and boundary conditions, describing the problem under consideration, are dimensionalized and the numerical solution is obtained by using the finite volume discretization methodology which is suitable for Fluid Mechanics applications. The numerical results for the velocity and temperature fields are shown in figures for different dimensionless parameters entering in the problem under consideration, such as the magnetic parameter, 
  M
   and the Grashof number, 
  Gr
  . This study predicts the effects of a constant magnetic field and uniform suction on the free convective flow of water near 4
  ℃
  , when the water is electrically conductive. Analysis of the results showed that the velocity and temperature profiles are noticeably influenced by these parameters.
   
     
    
 
</p></abstract><kwd-group><kwd>Free Convection; Water near 4℃; Constant Magnetic Field; Finite Volume Method</kwd></kwd-group></article-meta></front><body><sec id="s1"><title>1. Introduction</title><p>Free convection flow past an infinite vertical plate is an important application from a technological point of view. It becomes a more attractive problem when the fluid is water near 4˚C, electrically conductive, and the flow is subjected to a transverse and constant magnetic field.</p><p>It is known that for a fluid like air or water at ordinary temperature and atmospheric pressure the variation <img src="10-7401229\cd7c6ff1-6812-4322-8be2-67fba3ef2278.jpg" /> of the density with the variation <img src="10-7401229\35678f1f-f006-40ef-9fea-128aca844860.jpg" /> of the temperature is given by</p><disp-formula id="scirp.27131-formula19126"><label>(1)</label><graphic position="anchor" xlink:href="10-7401229\9a190f8c-8dc6-4b8a-b52a-d13eb393171c.jpg"  xlink:type="simple"/></disp-formula><p>where <img src="10-7401229\1e414bc0-7826-4b6e-9e80-6e6361ae5e40.jpg" /> at 20˚C. However, for temperature variations of magnitude &#177;4˚C away from 4˚C, the variations in density are very closely given by</p><disp-formula id="scirp.27131-formula19127"><label>(2)</label><graphic position="anchor" xlink:href="10-7401229\9379d5de-e50d-4fc5-a6c6-c110af3456ab.jpg"  xlink:type="simple"/></disp-formula><p>with <img src="10-7401229\2e29fa18-947f-4225-8983-8fd36786301d.jpg" /> equal to<img src="10-7401229\4abc70cc-99d6-473b-b6e3-8e23ab766984.jpg" />. From the above it is apparent that for small temperature variations, free convection in water near 4˚C would be different from that at 20˚C [<xref ref-type="bibr" rid="scirp.27131-ref1">1</xref>].</p><p>Many researchers have studied the steady free convective flow of water near 4˚C past a vertical plate. Govindarajulu [<xref ref-type="bibr" rid="scirp.27131-ref2">2</xref>] has studied the steady free convection flow of water near 4˚C on vertical and horizontal plates when the temperature of the plate is varying as a power of the distance along the plate from the leading edge. Soundalgekar [<xref ref-type="bibr" rid="scirp.27131-ref3">3</xref>] has investigated the free convection effects on oscillatory flow of water near 4˚C past an infinite vertical and porous plate with constant suction. The transient free convection of water near 4˚C over a doubly infinite vertical porous plate was studied by Pop and Raptis [<xref ref-type="bibr" rid="scirp.27131-ref4">4</xref>].</p><p>The combined convection flow of water near 4˚C through a porous medium bounded by a vertical plate was studied by Raptis and Pop [<xref ref-type="bibr" rid="scirp.27131-ref5">5</xref>]. Raptis and Perdikis also studied the free convection flow of water near 4˚C past an infinite porous plate with constant suction and free stream-velocity [<xref ref-type="bibr" rid="scirp.27131-ref6">6</xref>]. Singh and Raptis, further investigated the free-convection flow of water near 4˚C past an infinite vertical porous plate with constant heatflux [<xref ref-type="bibr" rid="scirp.27131-ref7">7</xref>]. The steady mixed convective water flow over a vertical plate in a porous medium near 4˚C when the wall temperature and surface heat flux vary, were studied by Ling et al. [8,9]. Oztop et al. [<xref ref-type="bibr" rid="scirp.27131-ref10">10</xref>], studied the natural convection in a triangular enclosure filled with porous media saturated with water near 4˚C. Recently, the free convection stagnation-point boundary-layer flow in a porous medium with density maximum was studied by Merkin and Kumaran [<xref ref-type="bibr" rid="scirp.27131-ref11">11</xref>]. The mixed convection of water near 4˚C along a wedge with variable surface temperature in porous medium was studied by Khan and Gorla [<xref ref-type="bibr" rid="scirp.27131-ref12">12</xref>]. They also studied the nonsimilar solutions for mixed convection of water near 4˚C in a porous medium [<xref ref-type="bibr" rid="scirp.27131-ref13">13</xref>].</p><p>The MHD free-convection effects on the oscillatory flow of water near 4˚C past an infinite porous plate was studied by Georgantopoulos et al. [<xref ref-type="bibr" rid="scirp.27131-ref14">14</xref>]. The steady Magnetohydrodynamic (MHD) free convective flow of water near 4˚C past a semi-infinite porous plate was studied by Perdikis and Takhar [<xref ref-type="bibr" rid="scirp.27131-ref15">15</xref>]. Recently, Guedda et al. [<xref ref-type="bibr" rid="scirp.27131-ref16">16</xref>], used the Chebyshev pseudospectral differentiation matrix (ChPDM) approach for studying the MHD mixed convection of a vertical plate embedded in a porous medium filled with water near 4˚C.</p><p>In this work we consider the unsteady free convective flow of water near 4˚C in the laminar boundary layer over a vertically moving permeable plate, under the influence of a constant transverse magnetic field. The presented results were obtained after dimensionalization of the PDEs using a numerical approach. This approach is based on the finite volume (FV) discretization scheme which is suitable for Fluid Mechanics applications. The discretization was performed with the help of a specialized symbolic package created by the authors in &#160;Mathematica.</p></sec><sec id="s2"><title>2. Mathematical Analysis</title><p>We consider the unsteady free convective and MHD flow of water near 4˚C past an infinite vertical moving plate with uniform suction. The <img src="10-7401229\0659f260-2296-4be6-9f81-203867d899c8.jpg" />-axis is taken along the plate in the vertical upward direction and the <img src="10-7401229\7bbaec83-1632-4224-9bb9-f3cb4fd42c9f.jpg" />-axis normal to the plate, <xref ref-type="fig" rid="fig1">Figure 1</xref>. The equations governing the problem are:</p><p>Continuity equation</p><disp-formula id="scirp.27131-formula19128"><label>(3)</label><graphic position="anchor" xlink:href="10-7401229\4bea8d2d-5489-4014-998b-e6f6f42610b5.jpg"  xlink:type="simple"/></disp-formula><p>Equation of motion</p><disp-formula id="scirp.27131-formula19129"><label>(4)</label><graphic position="anchor" xlink:href="10-7401229\9225461c-4d70-44dd-99b0-72b090e2981a.jpg"  xlink:type="simple"/></disp-formula><p>Energy equation</p><disp-formula id="scirp.27131-formula19130"><label>(5)</label><graphic position="anchor" xlink:href="10-7401229\5b7637dc-b9e0-43d0-b90b-c531e464e76b.jpg"  xlink:type="simple"/></disp-formula><p>where <img src="10-7401229\6103a5dd-aeaf-4b1b-9bd8-bce739362e44.jpg" /> is the velocity component at the <img src="10-7401229\e6a38cbd-4a97-4071-8ad2-7c1ee2f617ba.jpg" />-direction, <img src="10-7401229\2b988351-cb8d-4c04-8ba0-5f5db324989e.jpg" />is the normal velocity at the plate,<img src="10-7401229\30e632f7-9a24-4ed3-acfc-f00f04531416.jpg" />: the time;<img src="10-7401229\515e6095-cc7d-4974-8395-79dcc894f153.jpg" />: the acceleration due to gravity;<img src="10-7401229\78f010f4-cbe2-4e65-b210-e8a26799b75c.jpg" />: the coefficient of thermal expansion;<img src="10-7401229\2da2c562-71bd-4b6d-b255-e4372af6d648.jpg" />: the kinematic viscosity;<img src="10-7401229\f350fba4-c65b-405d-97ec-6289b5fb6cdb.jpg" />: the electrical conductivity;<img src="10-7401229\a858b59e-9bda-420e-aba9-e25d1ed077fe.jpg" />: the magnetic induction;<img src="10-7401229\641eb85d-86e5-4620-945d-9a6cb6cdc17c.jpg" />: the fluid density;<img src="10-7401229\4d1adf63-6171-4d51-b9e4-3f65c296cd8c.jpg" />: the fluid temperature;<img src="10-7401229\7592620a-217f-4210-9e4a-765685beb903.jpg" />: the</p><p>fluid temperature at infinity;<img src="10-7401229\8b74f2da-9ca6-4277-936d-9ad7e2f81360.jpg" />: the specific heat at constant pressure and<img src="10-7401229\7735b5dc-bd2a-4263-bb19-f874d82a21c0.jpg" />: the thermal conductivity.</p><p>The initial and the boundary conditions are</p><disp-formula id="scirp.27131-formula19131"><label>(6)</label><graphic position="anchor" xlink:href="10-7401229\929794fb-e539-4823-ab69-19d20d539b6c.jpg"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.27131-formula19132"><label>(7)</label><graphic position="anchor" xlink:href="10-7401229\b94a007d-ba57-4b8f-b75f-fc0f80fd77f3.jpg"  xlink:type="simple"/></disp-formula><p>where u<sub>0</sub> is the velocity of the plate, <img src="10-7401229\156bafc1-d638-4063-ab99-6b660565c50a.jpg" />is the constant normal suction and <img src="10-7401229\7f672874-f60b-41ca-bcc2-bc719ee3caba.jpg" /> is the temperature of the plate. From (3) it is obtained that<img src="10-7401229\23414dc6-0ff1-4679-9142-05b0fdb75ece.jpg" />, for every<img src="10-7401229\b0654184-450c-4544-8b9e-299d0380ef0a.jpg" />.</p><p>We introduce the dimensionless quantities</p><disp-formula id="scirp.27131-formula19133"><label>(8)</label><graphic position="anchor" xlink:href="10-7401229\351018f0-3a6c-458b-8fcb-8be994a2e9b7.jpg"  xlink:type="simple"/></disp-formula><p>Using the dimensionless quantities in (8), Equations (4) and (5) become respectively:</p><disp-formula id="scirp.27131-formula19134"><label>(9)</label><graphic position="anchor" xlink:href="10-7401229\52a971b0-cce1-4016-8ccb-05fb6d8f1358.jpg"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.27131-formula19135"><label>(10)</label><graphic position="anchor" xlink:href="10-7401229\cc5cf681-a1fa-4cf3-8ffa-e696535bb10f.jpg"  xlink:type="simple"/></disp-formula><p>The initial and boundary conditions in dimensionless form are as follows:</p><disp-formula id="scirp.27131-formula19136"><label>(11)</label><graphic position="anchor" xlink:href="10-7401229\ed6f6b33-b23a-4549-a60d-fd02c892c8d7.jpg"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.27131-formula19137"><label>(12)</label><graphic position="anchor" xlink:href="10-7401229\b7e2d55f-42ab-4af5-a16f-7c88dd4ff901.jpg"  xlink:type="simple"/></disp-formula><p>Finally, the problem under consideration is described by the system of Equations (9) and (10), subjected to the initial and boundary conditions (11) and (12).</p></sec><sec id="s3"><title>3. Numerical Solution</title><p>Contrary to the technique used in previous works of the authors for numerically solving the problem at hand [<xref ref-type="bibr" rid="scirp.27131-ref17">17</xref>], in the present paper we follow a more symbolic approach. For this purpose we have used the Computer Algebra System (CAS) Mathematica [<xref ref-type="bibr" rid="scirp.27131-ref18">18</xref>].</p><p>The analysis begins by obtaining the discretized form of the system of Equations (9)-(10) by using a symbolic package developed by the authors for that purpose. To discretize the coupled set of PDEs the finite volume method on a collocated grid is used (all variables are discretized at the center of the control volume, <xref ref-type="fig" rid="fig2">Figure 2</xref>) [<xref ref-type="bibr" rid="scirp.27131-ref19">19</xref>]. The result of this discretization is given below:</p><disp-formula id="scirp.27131-formula19138"><label>(13)</label><graphic position="anchor" xlink:href="10-7401229\a2403f24-e749-4bb8-8632-9a9dc64b9c82.jpg"  xlink:type="simple"/></disp-formula><disp-formula id="scirp.27131-formula19139"><label>(14)</label><graphic position="anchor" xlink:href="10-7401229\e996d8c6-b180-4d9d-956f-ab9d397e2dad.jpg"  xlink:type="simple"/></disp-formula><p>where <img src="10-7401229\ded03b46-60bf-4146-93ad-6c93e83e5b4d.jpg" /> and <img src="10-7401229\199435bb-9fe6-49ce-bfbf-de76783ada15.jpg" /> are the unknown quantities at the center of the control volume as shown in <xref ref-type="fig" rid="fig2">Figure 2</xref>, <img src="10-7401229\0e149af4-580e-46f4-aeda-c555062e6a18.jpg" />and <img src="10-7401229\70fbc09a-59b9-4edb-ac6b-4448d7a33741.jpg" /> are the unknown quantities at the center of the control volume at the previous time, and where all the parameters, <img src="10-7401229\06a378b3-bbd5-4270-9d96-047e0e56153a.jpg" />, <img src="10-7401229\f1225c25-c7b4-4b1a-8c9c-c26e3604bb82.jpg" />and <img src="10-7401229\1590cc70-a72c-4a1b-898a-7807afdb716e.jpg" /> are introduced in (8).</p><p>Having obtained the discretized systems (13)-(14), we construct the system of algebraic equations that constitute the grid for each time step. By grid and time in-</p><p>dependence studies with different grid sizes, it is established that the results are time and space independent for <img src="10-7401229\f98ed3fd-94f1-475f-bea6-b02ec4629f30.jpg" /> equal to 0.05 and <img src="10-7401229\5f8c26b2-f2ef-4e00-afe9-0441f7dc8846.jpg" /> equal to<img src="10-7401229\fe99f5d3-180f-4422-85ee-deec4e133ffd.jpg" />.</p><p>Then, for each time step, the system is solved algebraically by Mathematica’s function Solve in respect to the grid values of the functions<img src="10-7401229\673f1b81-12ec-4a47-8ca2-c7bb9e99ec14.jpg" />, after first substituting the values of the previous time steps to the system. The procedure is optimized for speed by keeping all the grid values for all the time steps in memory.</p></sec><sec id="s4"><title>4. Results and Discussion</title><p>The system of equations under consideration is a highly coupled system of two nonlinear equations, whose solution can be tedious. However, with the advancement of numerical techniques such as the finite volume (FV) methodology, which is suitable for Fluid Mechanics applications, problems like this can be solved. A thorough analysis of the problem under consideration includes the study of the velocity and temperature fields under the influence of the dimensionless parameters entering in the problem, such as the magnetic parameter, <img src="10-7401229\b5046c6a-2b2c-489c-b70c-814fd7ab0a2c.jpg" />and the Grashof number,<img src="10-7401229\815468a6-6eb2-408e-9d0e-8aa2352cfef9.jpg" />. The Prandtl number was the same for all cases and equal to 11.4.</p><p>Initially, the suction velocity was considered equal to zero, <img src="10-7401229\2934043c-41b3-49ee-ba6c-8dd9ffbb27ed.jpg" />and the influence of the dimensionless parameters entering in the problem was studied. Next, the effect of a constant suction velocity, <img src="10-7401229\d4b34984-5df9-4242-afc6-be4cff299e11.jpg" />, on the velocity and temperature profiles under the influence of a constant transverse magnetic field was investigated.</p><sec id="s4_1"><title>4.1. Case I, Suction Velocity, <img src="10-7401229\627144ea-6993-4fa3-9cea-960786ae030e.jpg" />, Is Zero</title><p>The velocity and temperature distributions for different dimensionless times <img src="10-7401229\d6f1de91-a26b-4482-8ea6-8ae833932449.jpg" /> are shown in <xref ref-type="fig" rid="fig3">Figure 3</xref>. In this case, the velocity and temperature fields increase away from the flat plate, as time increases.</p><p>The effect of the magnetic parameter, M, on the</p><p>velocity field for different times<img src="10-7401229\39b2b6b4-f463-4541-a355-d473e27ffba7.jpg" />, (<img src="10-7401229\b722858d-a54e-4bdf-95e7-7be187c33eaf.jpg" />and<img src="10-7401229\5807a7d6-1b87-461a-985e-bd7cc1ccaff9.jpg" />) are shown in Figures 4 and 5. For <img src="10-7401229\b68c395e-c678-4c08-b9e9-7a9c692d5fe3.jpg" /> the magnetic parameter, M, decreases the velocity, <xref ref-type="fig" rid="fig4">Figure 4</xref>. Similarly, for t = 0.25 the velocity decreased throughout the boundary layer when the magnetic parameter was increased, <xref ref-type="fig" rid="fig5">Figure 5</xref>. This is because the presence of a magnetic field introduces a force (Lorentz force) that acts on the fluid (water) creating a drag-like effect that slows down the flow in the boundary layer.</p><p>Figures 6 and 7 show the effect of Grashof number, <img src="10-7401229\b5cf98bd-cd32-4d4b-ac29-0b2bea9d7eb2.jpg" />, on the velocity profiles for <img src="10-7401229\29ffd709-66ce-43c4-b1e6-27c920aa1fc7.jpg" /> and<img src="10-7401229\7390cfae-127e-43d2-95e1-d1e330b2f6d0.jpg" />. The velocity increased noticeably near the plate as the Grashof number increased, due to the increase of the buoyancy forces compared to the viscous forces acting on the fluid (water) near 4˚C.</p></sec><sec id="s4_2"><title>4.2. Case II, Suction Velocity, <img src="10-7401229\27ca0eeb-7068-4c49-9003-7c11042e3ee9.jpg" />, Is Constant</title><p>The effect of a constant suction velocity on the velocity and temperature fields under the influence of a constant transverse magnetic field was also studied. The effects of suction velocity upon the velocity and temperature fields for dimensionless time t = 0.25 are shown in Figures 8</p><p>and 9. It is evident from the figures that as the absolute value of suction velocity increases, the profiles of the velocity and temperature decrease. These findings are in accordance with previously published results [<xref ref-type="bibr" rid="scirp.27131-ref20">20</xref>]. It is also worth noting that the suction velocity has a more profound effect on the temperature field, <xref ref-type="fig" rid="fig9">Figure 9</xref>.</p></sec></sec><sec id="s5"><title>5. Conclusions</title><p>The unsteady free convective flow of water near 4˚C, past a vertical plate, moving with constant velocity, and subjected to a transverse magnetic field and constant suction velocity was numerically studied.</p><p>In the present paper an analytic/symbolic approach was chosen for solving the system of Equations (9) and (10), subjected to the initial and boundary conditions (11)</p><p>and (12). A symbolic package developed in Mathematica is used for obtaining the discretization of the problem and for constructing the algebraic system to be solved for each grid point. Then, for each time step the system was solved analytically using the numerical data of the previous time step, hence avoiding errors in accuracy due to the use of a numerical solver such as a Newton-like method. As a consequence, the obtained solution is more accurate for greater values of t.</p><p>Moreover, further development of the symbolic package for the fast and accurate discretization of dynamical systems using the Finite Volume approach (with the option of different grid choices available to the user) will be an invaluable tool for any researcher using the Finite Volumes discretization scheme, especially for systems in multi-dimensions where the calculations by hand are not only time consuming but also error prone.</p><p>The results of this study showed that the velocity and temperature fields increase away from the flat plate, as time increases. For<img src="10-7401229\aee0a0ae-d6af-4282-914e-1e802edd74b8.jpg" />, the velocity decreased throughout the boundary layer when the magnetic parameter was increased while it increased noticeably near the plate when the Grashof number was increased. Finally, as the value of the suction velocity increased, the profiles of velocity and temperature decreased.</p></sec><sec id="s6"><title>REFERENCES</title></sec><sec id="s7"><title>NOTES</title></sec></body><back><ref-list><title>References</title><ref id="scirp.27131-ref1"><label>1</label><mixed-citation publication-type="other" xlink:type="simple">S. Goren, “On Free Convection in Water at 4℃,” Chemical Engineering Science, Vol. 21, No. 6-7, 1966, pp. 515-518. doi:10.1016/0009-2509(66)85065-0</mixed-citation></ref><ref id="scirp.27131-ref2"><label>2</label><mixed-citation publication-type="other" xlink:type="simple">T. Govindarajulu, “Free Convection Flow of Water at 4℃ on Vertical and Horizontal Plates,” Chemical Engineering Science, Vol. 25, No. 11, 1970, pp. 1827-1828. 
doi:10.1016/0009-2509(70)80076-8</mixed-citation></ref><ref id="scirp.27131-ref3"><label>3</label><mixed-citation publication-type="other" xlink:type="simple">V. Soundalgekar, “Free Convection Effects on the Oscillatory Flow of Water at 4℃ past an Infinite Vertical, Porous Plate with Constant Suction,” Heat and Mass Transfer, Vol. 9, 1976, pp. 111-115.</mixed-citation></ref><ref id="scirp.27131-ref4"><label>4</label><mixed-citation publication-type="other" xlink:type="simple">I. Pop and A. Raptis, “A Note on Transient Free Convection of Water at 4℃ over a Doubly Infinite Vertical Porous Plate,” Journal of Heat Transfer-Transactions of the ASME, Vol. 104, 1982, pp. 800-802. 
doi:10.1115/1.3245206</mixed-citation></ref><ref id="scirp.27131-ref5"><label>5</label><mixed-citation publication-type="other" xlink:type="simple">A. Raptis and I. Pop, “Combined Convection Flow of Water at 4℃ through a Porous Medium Bounded by a Vertical Surface,” Letters in Heat and Mass Transfer, Vol. 9, 1982, pp. 309-318.  
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